A dataset provided by the European Space Agency

Name 040518
Title X-ray follow-up observations of known transient INTEGRAL sources
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405180501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405181901
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405182701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405183801

DOI 10.5270/esa-msb2apq
Author Dr Lara Sidoli
Description We propose to trigger a maximum of 5 XMM follow-up observations on known transient sources discovered with INTEGRAL Observatory,if they undergo a new outburst during AO5. We ask for 20 ks per observation,usign EPIC PN as primary instrument, in order to get a high-quality X-ray spectrum.XMM spectral and spatial capabilities are essential in unveiling their nature (still unknown for the select targets), and in refining their sky positions, enabling multiwavelength follow-up observations.
Publication An alternative hypothesis for the outburst mechanism in supergiant fast X-ray transients: the case of IGR J11215-5952 . Sidoli, L., Romano, P., et all. . A&A . 476-1307 . 2007 . 2007A&A...476.1307S ,
The XMM-Newton view of supergiant fast X-ray transients: the case of IGR J16418-4532 . Sidoli, L., Mereghetti, S., et all. . MNRAS . 420-554 . 2012 . 2012MNRAS.420..554S ,
XMM-Newton and INTEGRAL observations of the very faint X-ray transient IGR J17285-2922-XTE J1728-295 during the 2010 outburst . Sidoli, L., Paizis, A., et all. . MNRAS . 415-2373 . 2011 . 2011MNRAS.415.2373S ,
General X-ray properties of hot, massive stars . Naze, Yael, . BSRSL . 80-109 . 2011 . 2011BSRSL..80..109N ,
Exospheric solar wind charge exchange as seen by XMM-Newton . Carter, J. A., Semba, S., . AN . 333-313 . 2012 . 2012AN....333..313C ,
Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog . Lin, Dacheng, Webb, Natalie A., . ApJ . 756-27 . 2012 . 2012ApJ...756...27L ,
Automatic Classification of Time-variable X-Ray Sources . Lo, Kitty K., Farrell, Sean, et all. . ApJ . 786-20 . 2014 . 2014ApJ...786...20L ,
The diversity of quasars unified by accretion and orientation . Shen, Yue, Ho, Luis C., . Natur . 513-210 . 2014 . 2014Natur.513..210S ,
Serendipitous UV source catalogues for 10 yea...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2007-02-09T16:23:25Z/2011-02-24T00:32:26Z
Version 17.56_20190403_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations.
Since Earth's atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
Creator Contact https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published 2012-03-15T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2012-03-15T00:00:00Z, 040518, 17.56_20190403_1200. https://doi.org/10.5270/esa-msb2apq